Titlebook: Literature 1997, Part 1; G. Burkhardt,U. Esser,G. Zech Book 1998 Springer-Verlag Berlin Heidelberg 1998 Celestial mechanics.astronomy.astr

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Lasting

Theoretical Astrophysics order to show this effect for some relevant and representative examples of unified gauge models, the authors have chosen SO(10), and SU(5)., SO(10). with a particular scheme for fermion masses (DHR model). The analysis has been performed for two choices of neutrinos parameters, predicted by the abo

NUL

Sunphotospheric lines applied to a large number of Ca II K targets yield some average results: These magnetic features are 2 to 3 arcsec in diameter, dark at disk center and bright at the limb. Their magnetic field strength is typically 1400 G, with the field vertically oriented on average. Their magne

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